Abstract

The work described here makes it possible to identify anomalous wind behavior such as the nighttime meridional wind abatements that occur at F‐region heights. A new analysis technique uses a simple empirical wind model to simulate measurements of “normal” winds (as measured by the Neutral Atmosphere and Temperature Experiment (NATE) that flew on the Atmosphere Explorer‐E (AE‐E)) to highlight anomalous wind measurements made by the satellite while in circular orbits at 270–290 km altitude. Our approach is based on the recognition that the “in orbit” wind variation must show the combined effects of the diurnal wind variation as seen from the ground with the latitude variation of the satellite orbit. For the data period 77250–78035 examined thus far, the wind abatement always occurred with a corresponding pressure or temperature maximum, and was detected on 12 out of the 36 nights with data. This study has revealed that the wind abatements occur only during or shortly after increases in solar EUV flux, as indicated by daily radio flux measurements. In the past, nighttime wind reversals at mid‐latitudes have been associated with increased geomagnetic activity. This study indicates that intensified solar EUV heating may be responsible for anomalous thermospheric nighttime winds at mid‐latitudes.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.